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| '''The meeting will address the evolution of the protoplanetary disks at the decoupling stage. The goal is to focus on: ''' | . The meeting will address the evolution of the protoplanetary disks at the decoupling stage. The goal is to focus on: * the possible formation of gaseous structures in the protoplanetary disks, particularly in the dead-zone, under various instabilities (baroclinic, or via Rossby or edge modes) * their lifetime and evolution (stability, migration, collisions ....), * their ability to capture the solid material and to survive once loaded. |
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| * '''the possible formation of gaseous structures in the protoplanetary disks, particularly in the dead-zone, under various instabilities (baroclinic, or via Rossby or edge modes) ''' * '''their lifetime and evolution (stability, migration, collisions ....), ''' * '''their ability to capture the solid material and to survive once loaded. ''' '''Emphasis will be placed on the hydrodynamical aspects of the problem, without and with self-gravity, but MHD processes will not be forgotten. We will look also at the links with the experimental and numerical works performed in the physics of rotating flows and granular media.''' |
Emphasis will be placed on the hydrodynamical aspects of the problem, without and with self-gravity, but MHD processes will not be forgotten. We will look also at the links with the experimental and numerical works performed in the physics of rotating flows and granular media. |
"Instabilities and Structures in Proto-Planetary disks"
A workshop in planet formation Marseille France
Dates: 17th - 20th september 2012
Location: Marseille city - France
Rationale:
- The meeting will address the evolution of the protoplanetary disks at the decoupling stage. The goal is to focus on: * the possible formation of gaseous structures in the protoplanetary disks, particularly in the dead-zone, under various instabilities (baroclinic, or via Rossby or edge modes)
- their lifetime and evolution (stability, migration, collisions ....),
- their ability to capture the solid material and to survive once loaded.
Emphasis will be placed on the hydrodynamical aspects of the problem, without and with self-gravity, but MHD processes will not be forgotten. We will look also at the links with the experimental and numerical works performed in the physics of rotating flows and granular media.